We used the online tool Virtual Observatory SED Analyser (VOSA)http://svo2.cab.inta-csic.es/theory/vosa., developed by the Spanish Virtual Observatory, to automatically compile photometry from the UV to the IR from the available catalogs in the Virtual Observatoryhttp://svo2.cab.inta-csic.es/theory/vosa/help.php?what=creditscredits:vophot. In addition to the new Gaia EDR3 photometry [1]}, we included data from GALEXGalaxy Evolution Explorer [2]}, APASSAAVSO Photometric All-Sky Survey 9 [3]}, the Stroemgren-Crawford uvby\(\beta \)  photometry catalog [4]}, 2MASSTwo Micron All-Sky Survey [5]}, WISEWide-Field Infrared Survey Explore [6]}; IRASInfrared Astronomical Satellite [7]}, Spitzer [8]}, and AKARI ([9]}; [10]}), among others. Information about the quality of the photometry is available in the catalogs, and the photometric points with poor-quality flags were discarded. Additional UBVRI and L,M photometry was extracted when necessary ([11]}, [12]}, [13]}; [14]}; [15]}, [16]} and [17]}). Fluxes at millimeter wavelengths were also used in this work, as indicated in Sect. REF .
